基于轨道观测的月球年轻撞击坑中物质状态的估计

M. Shpekin, R. Ferreyra
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引用次数: 0

摘要

. 该报告根据从月球轨道获得的高分辨率图像,对年轻撞击坑的地形进行了3d调查。被检查的陨石坑包括:月球背面的齐奥尔科夫斯基陨石坑和艾特肯陨石坑,可见半球的提丘陨石坑和伊娜陨石坑,以及月球边缘地带的东方海陨石坑。为了建立3d模型,使用了苏联航天器“zone -6,-8”和美国航天器“阿波罗-17”的轨道图像,以及从月球侦察轨道器(LRO)传输到地球的图像。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Estimation of the state of matter in young impact craters on the Moon based on the orbital observations
. The report examines the results of a 3D-survey of the relief in young impact craters based on high-resolution images obtained from lunar orbits. The craters examined included: the Tsiolkovsky and Aitken craters on the far side of the Moon, the Ticho and Ina craters of the visible hemisphere, as well as the Orientale Mare in the marginal zone of the Moon. To build 3D-models, orbital images of the Soviet spacecraft ” Zond-6,-8 ” and the American spacecraft “ Apollo-17 ” delivered to Earth, as well as images transmitted to Earth from the Lunar Reconnaissance Orbiter (LRO) were used.
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